a grain level model for the study of failure initiation and ......cohesive elements as an approach...
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A grain level model for the study of failure initiationand evolution in polycrystalline brittle materials. Part
II: Numerical examples
Horacio D. Espinosa *, Pablo D. Zavattieri 1
Department of Mechanical Engineering, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208-3111, USA
Received 17 September 2001; received in revised form 11 April 2002
Abstract
Numerical aspects of the grain level micromechanical model presented in part I are discussed in this study. They
include, an examination of solution convergence in the context of cohesive elements used as an approach to model
crack initiation and propagation; performance of parametric studies to assess the role of grain boundary strength
and toughness, and their stochasticity, on damage initiation and evolution. Simulations of wave propagation ex-
periments, performed on alumina, are used to illustrate the capabilities of the model in the framework of experi-
mental measurements. The solution convergence studies show that when the length of the cohesive elements is
smaller than the cohesive zone size and when the initial slope of the traction-separation cohesive law is properly
chosen, the predictions concerning microcrack initiation and evolution are mesh independent. Other features ex-
amined in the simulations were the effect of initial stresses and defects resulting from the material manufactur-
ing process. Also described are conditions on the selection of the representative volume element size, as a function
of ceramic properties, to capture the proper distance between crack initiation sites. Crack branching is predicted in
the case of strong ceramics and sufficient distance between nucleation sites. Rate effects in the extension of mi-
crocracks were studied in the context of damage kinetics and fragmentation patterns. The simulations show that
crack speed can be significantly varied in the presence of rate effects and as a result crack diffusion by nucleation of
multiple sites achieved. This paper illustrates the utilization of grain level models to predict material constitutive
behavior in the presence, or absence, of initial defects resulting from material manufacturing. Likewise, these models
can be employed in the design of novel heterogeneous materials with hierarchical microstructures, multi-phases and/
or layers.
� 2002 Elsevier Science Ltd. All rights reserved.
1. Introduction
The grain level micromechanical model pre-sented in part I is used to analyze the evolution of
damage in ceramics when they are subjected to
stress pulses that are large enough in amplitude to
initiate microcracks, but short enough in duration
* Corresponding author. Tel.: +847-467-5989; fax: +847-491-
3915.
E-mail address: [email protected] (H.D. Espin-
osa).
URL: http://www.mech.northwestern.edu/espinosa.1 Present address: General Motors Research and Develop-
ment Center, 30500 Mound Road, Warren, MI 48090-9055,
USA.
0167-6636/03/$ - see front matter � 2002 Elsevier Science Ltd. All rights reserved.
PII: S0167-6636 (02 )00287-9
Mechanics of Materials 35 (2003) 365–394
www.elsevier.com/locate/mechmat
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to prevent their coalescence into macrocracks.
Since failure processes in ceramics are transient in
nature, even under nominally quasi-static loading
conditions, inertia effects play an important role.
Normal plate impact experiments have proved to
be successful in inducing microcracking in aluminaunder well-known and controlled loading condi-
tions without causing macroscopic failure of the
material (Raiser et al., 1990, 1994; Raiser, 1993;
Espinosa, 1992; Espinosa et al., 1992). This ex-
periment uses an eight pointed star-shaped flyer
plate that impacts a square ceramic specimen,
subjecting the central octagonal region to a plane
pulse. Fig. 1 shows the soft-recovery normal im-pact configuration. A tensile pulse is originated,
from an intentional gap manufactured between the
specimen and the momentum trap, upon reflection
of the compressive pulse.
A detailed study of the damage kinetics in these
experiments was recently carried out by Zavattieri
and Espinosa (2001). The interferometrically
measured velocity profiles obtained from these
experiments, which are very rich in information
concerning damage initiation and kinetics as well
as postmortem SEM and TEM observations,
make this experiment an ideal candidate for the
analysis of material failure in conjunction with theproposed grain level micromechanical model un-
der a fully dynamic framework. The experiments
and simulations not only allow identification of
model parameters but also explain the different
failure mechanisms of ceramics as a function of
microstructure morphology and grain boundary
chemistry.
Analyzing the time history of failure is moreimportant than simply examining the final out-
come. While postmortem observations can reveal
failure mechanisms such as inter-granular and
transgranular fractures and their relative pro-
portions, they do not indicate the sequential
order of the events or the conditions for crack
initiation. Additionally, postmortem observations
do not provide sufficient information about mi-crofracture nor evolution of stress-carrying ca-
pacity.
The focus of this contribution is in the numer-
ical aspects of the proposed grain level microme-
chanical model. To illustrate the capabilities of the
model, the normal impact experiments performed
on Al2O3 by Raiser et al. (1990) and Espinosa
(1992) are studied while focusing on the effects ofinterface element parameters, grain anisotropy,
grain size, and stochastic distribution of grain
boundary properties. The paper starts with the
definition of computational cell, boundary and
initial conditions. A section is devoted to the
analysis of solution convergence in the context of
cohesive elements as an approach to model crack
initiation and propagation. A parametric analysisis conducted to examine the effect of representative
volume element (RVE) size and cohesive element
properties on damage evolution. The effect of ini-
tial microcracks, resulting from the sintering pro-
cess, grain boundary strength, and rate dependent
microcracking are investigated in various subsec-
tions. The effect of crack initiation distance on
propagation and branching is also examined inceramics with strong grain boundaries, i.e., high
purity ceramics.Fig. 1. Soft-recovery normal impact configuration.
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2. Definition of computational cell
A RVE of an actual microstructure is consid-
ered for the analysis. An elastic-anisotropic model
for the grains, incorporating grain anisotropy, isused under plane strain conditions. Cohesive in-
terface elements are embedded along grain
boundaries to simulate microcrack initiation and
evolution. The normal and shear traction compo-
nents in the interface elements are calculated from
the interface cohesive laws presented in part I of
this work. The grain morphology is represented by
either digitizing a real ceramic microstructure or
automatically generating a Voronoi Tessellation.
In view of the uniaxial strain conditions pre-
vailing in the specimen and assuming periodicity, a
RVE of only part of the ceramic specimen is
considered. Fig. 2(a) shows a strip of the experi-mental configuration: flyer, momentum trap, and
specimen plates are considered in the analysis.
Furthermore, for the low impact velocities con-
sidered in these simulations, only a small portion
of the ceramic plate, in the spall region, is simu-
lated. The dimensions of the cell are L� H . This
Fig. 2. (a) Schematics of the computational cell used in the analyses. (b) Schematic of boundary conditions employed in the analyses.
H.D. Espinosa, P.D. Zavattieri / Mechanics of Materials 35 (2003) 365–394 367
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feature is consistent with experimental observa-
tions showing that damage and inelasticity, at
impact velocities below 100 m/s, are restricted to
the spall region.
3. Boundary and initial conditions
Assuming that the computational cell is re-
peated in the x-direction, the following periodic
boundary conditions are applied
uð0; y; tÞ ¼ uðL; y; tÞ; vð0; y; tÞ ¼ vðL; y; tÞ;að0; y; tÞ ¼ aðL; y; tÞ ð1Þ
where L is the width of the cell, u, v and a are the
displacement, velocity and acceleration vector
fields. Grains with nodes at x ¼ 0 have the same
principal material directions as the grains with
nodes at x ¼ L to ensure periodicity. Further-more, assuming that there is no damage in the
ceramic, except in the spall region where it re-
mains elastic throughout the deformation process,
the computational effort can be minimized by
replacing the rest of the ceramic with viscous
boundary conditions based on one dimensional
elastic wave theory, as discussed in part I. Con-
servation of momentum and continuity of veloc-ities and tractions lead to the following equations
for traction components tx and ty at y ¼ H and
y ¼ 0, namely,
txðx;H ; tÞ ¼ ðqcsÞcvxðx;H ; tÞ ð2Þ
tyðx;H ; tÞ ¼ ðqclÞc½vyðx;H ; tÞ � 2v1y � ð3Þ
txðx; 0; tÞ ¼ ðqcsÞcvxðx; 0; tÞ ð4Þ
tyðx; 0; tÞ ¼ ðqclÞcvyðx; 0; tÞ ð5Þwhere ð Þc are ceramic quantities, cl and cs are
longitudinal and shear wave speeds, q is the spe-
cific material density, vx and vy are the transverse
and normal velocities at the top of the RVE and v1y
is the normal velocity at the flyer-specimen inter-
face, which can be computed from the impact ve-
locity V0 by
v1y ¼
ðqclÞf
ðqclÞs þ ðqclÞf
V0 ð6Þ
in which ðqclÞf is longitudinal impedance of the
flyer. Here the reference point 1 is at the flyer-
specimen interface, and the normal traction on this
interface is given by t1y ¼ �2ðqclÞcv1y .
The initial transverse and normal velocities atthe bottom of the RVE are set to zero and at the
top of the RVE are given by
vxðx;H ; 0Þ ¼ 0 ð7Þ
vyðx;H ; 0Þ ¼ v1y ð8Þ
As discussed earlier, since the RVE is muchsmaller than the actual thickness of the ceramic,
special care must be taken at the boundaries to
include the reflection of the waves from free sur-
faces and the contact with the momentum trap
plate upon closure of the gap. The traction at the
top of the RVE, which is given by Eq. (3), is used
to simulate the compressive wave generated at the
flyer-specimen interface until the unloading of thewave reaches that point. Assuming that there is no
damage in compression, the duration of the first
compressive pulse can be reduced in the simula-
tions. Fig. 2(b) shows the Lagrangian X–t diagram
corresponding to the wave history, at the bound-
ary of the RVE, for the normal plate impact ex-
periments. In this diagram, Ls represents the
thickness of the specimen and LRVE representsthe height, i.e., H , of the RVE considered in the
analysis. Since the duration of the first compres-
sive pulse inside the specimen is Dt, the traction is
removed at t ¼ Dt to account for the unloading
originated at the flyer plate. The compressive
traction at the bottom of the RVE is given by Eq.
(5). Right after the first compression wave reaches
the bottom of the RVE, the unloading from theback of the specimen is represented by new viscous
boundary conditions at time t1. In order to simu-
late this wave reflection, the normal traction at
y ¼ 0 is modified to include such information. The
time at which this traction is applied is t1 ¼ Dt. In
this way, the spall plane is located at the middle of
the RVE. The contact with the momentum trap
occurs at t1 þ dt, where dt is the duration of theunloading pulse. This second pulse then travels
through the RVE and becomes tensile. Since this
second pulse is modified by microcracking, the
traction at the top of the RVE is recorded and
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stored so that it can be used to simulate its re-
flection at the impact surface (see Fig. 2(b) state 4
on the right).
The velocity vyðx; 0; tÞ at the bottom of the RVE
can be directly compared with the experimental
velocity history if two important features are takeninto account:
1. The velocity is corrected according to the im-
pedances of the specimen and momentum trap.
The velocity at the specimen-momentum trap
interface vfy (after contact) is given by vf
y ¼2ðqclÞsvyðx; 0; tÞ=ððqclÞMT þ ðqclÞsÞ, where ð Þs
and ð ÞMT denote specimen and momentum trapquantities, respectively. Considering that the ve-
locity at the back of the momentum trap is
twice vfy , this correction is given by
vy ¼4ðqclÞs
ðqclÞMT þ ðqclÞs
vyðx; 0; tÞ ð9Þ
2. The time at which waves arrive to the back ofthe momentum trap is different to the one in
the simulation due to the simplifications of the
model (i.e., the reduction of the duration of
the compression wave, etc.). The effect can be
taken into account exactly by using pulse dura-
tions, longitudinal wave speeds and width of
plates and RVE.
The material properties of the ceramic specimen
(Al2O3) are given in Table 1. The nonzero com-
ponents are denoted by only two indices (i.e.,
C1111 ¼ C11, C2222 ¼ C22, C1122 ¼ C12, C1212 ¼ C44,
etc.). It should be noted that alumina is a trigonal
system with only three planes of symmetry with
normals that do not coincide with the local axes of
co-ordinates except for axis 1. In terms of the
elastic constitutive matrix bCCIJ , this means thatC14 ¼ �C24 ¼ C45 6¼ 0 (Hearmon, 1956). In order
to perform plane strain analyses, the behavior of
alumina is assumed to be transversely isotropic (or
hexagonal) making C14 ¼ 0. Other mechanical
material parameters needed for this analysis are
wave speeds, impedances and densities of the dif-
ferent materials used in the experiments, which are
given in Table 2.
4. Solution convergence analysis
In addition to the usual requirements of mesh
independence, two other factors influence the so-
lution convergence of this grain level microme-
chanical model.First, the finite element size must be small en-
ough to accurately resolve the stress distribution in
the cohesive zone at microcrack tips. For a linearly
softening cohesive law, an approximation of the
cohesive zone size dcz at the crack tip is given by
Rice (1968) as
dcz p2
Eð1 � m2Þ
GIc
T 2max
¼ p2
KIC
Tmax
� �2
ð10Þ
Table 1
Material properties for alumina
Specimen properties: anisotropic
elastic constant for alumina Al2O3
Al2O3 (GPa)
(Hearmon, 1956)
C11 ¼ C22 465
C12 124
C13 ¼ C23 117
C14 ¼ �C24 101
C33 563
C44 ¼ 12ðC11 � C12Þ
C55 ¼ C66 233
Table 2
Properties of the different materials used in the experiments
Material Longitudinal
wave speed cl,
mm/ls
Transverse wave
speed cs, mm/ls
Acoustic imped-
ance, qcl GPa/mm/
ls
Shear imped-
ance, qcs GPa/
mm/ls
Mass density, q,
kg/m3
1018 CR 5.9 3.2 45.50 24.70 7700
Hampden 5.9 3.2 47.03 25.66 7861
Al6061-T6 6.4 3.0 17.34 8.23 2700
Ti6Al4V 6.2 3.1 27.71 13.96 4430
Al2O3 10.8 6.4 43.09 25.54 3990
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where m is the Poisson�s ratio, GIc and KIC are the
critical energy release rate and the fracture tough-
ness of the material in mode I, respectively. In order
to resolve the cohesive zone field, it is necessary for
the maximum interface element size, hc, inside thecohesive zone, to satisfy the following inequality:
hc � dcz ð11ÞThe second constraint for solution convergence
is related to the initial slope of the cohesive law,
see part I of this work. According to the traction-
separation relationship, this slope is given as
s ¼ Tmax
kcrdð12Þ
This initial slope works as a penalty parameter. As
the parameter grows, the solution improves.
Hence, it has to be large enough to be effective but
not so large as to provoke numerical instabilities.
According to Eq. (42) of part I, the element size
must satisfy the following inequality:
kcr �ThEd
ð13Þ
where h is the size of the triangular element. Since
we are using two linear interface elements on each
edge of the triangular element, h ¼ 2hc. For a gi-
ven element size, the parameter kcr can be chosen
in order to satisfy Eq. (13). However, it should be
noted that the critical effective displacement jumpcannot exceed unity, kcr 6 1; therefore, the maxi-
mum separation d would be limited by the fol-
lowing expression:
dP Tmax=s ð14ÞThis means that for a given slope and Tmax, the
maximum separation and, therefore, the area be-low the curve, cannot exceed a certain value.
Moreover, it is desired that
kcr � 1 ð15ÞNote that Eq. (13) can also be written in the
following way:
h � kcr
ETmax
d ð16Þ
According to this equation, the higher Tmax, the
smaller the element should be unless the critical
energy release rate (or d) is increased.
Typical values of dcz and h can be obtained for
different Tmax–KIC pairs. For instance, for Tmax ¼ 1
GPa and KIC ¼ 1 MPa m1=2 the cohesive zone is
dcz ¼ 1:57 lm and the required element size ac-
cording to Eq. (16) is hc ¼ h=2 � 1:41 lm for a
minimum slope of 200 GPa/lm. Hence, hc must be�1.41 and �1.57 lm according to Eq. (11). It
should be noted that the above minimum slope
s ¼ Tmax=d corresponds to kcr ¼ 1. In practice, it is
desirable to have kcr � 1 if the slope and element
size are to be optimum. For the previous example,
if kcr ¼ 0:1 is considered the minimum slope is
s ¼ 2000 GPa/lm and the required element size is
about h ¼ 0:14 lm, which easily satisfies Eq. (11).As previously noticed, the maximum allowable
element size becomes smaller for higher values of
Tmax. In fact, for Tmax ¼ 10 GPa and KIC ¼ 2
MPa m1=2 the cohesive zone is dcz ¼ 0:06 lm and
the required element size is hc ¼ 0:06 lm for a
minimum slope of 5500 GPa/lm and kcr ¼ 0:1.
The above analysis shows that elements smaller
than 0.1 lm are needed for microstructures withinterfacial strength as high as Tmax ¼ E=40. Like-
wise, kcr must be selected such that Eq. (13) is also
satisfied!
Fig. 3(a) shows the finite element meshes
utilized to study the solution convergence for a
Voronoi microstructures. In this case, a RVE of
20 � 20 lm with a grain size GS ¼ 2 lm, is
generated. The boundary conditions are appliedaccording to the previous section, the impact
velocity is V0 ¼ 90 m/s and the tensile pulse du-
ration is dt ¼ 40 ns. Several meshes are consid-
ered having the following element sizes: h ¼ 2, 1,
0.5, 0.25, 0.1, and 0.05 lm. Due to the number
of elements in the finest mesh (130,000 ele-
ments), Fig. 3(b) only shows that various mesh
refinements in one of the grains of the micro-structures.
Fig. 4 illustrates the stress distribution for the
six meshes. The interfacial parameters used for this
simulation are Tmax ¼ 10 GPa and KIC ¼ 2
MPa m1=2. It should be noted that the stress con-
centration becomes more significant for the finest
mesh as expected. Microcracking did not occur in
any case, even for the finest mesh, because of thehigh value of interfacial strength used in these
simulations. The distribution of effective stress is
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similar for the meshes with h ¼ 0:1 and 0.05 lm
indicating solution convergence.
Another interesting result showing the effect of
stress concentration due to a distribution of initial
defects, can be seen in Fig. 5. Also in this case a
similarity in the stress distribution can be observed
for the two most refined meshes. Figs. 4 and 5 are
snapshots of the microstructures at 3.5 ns, right
after the tensile pulse is generated in the middle of
the RVE.
Fig. 3. (a) Geometry with 10 � 10 grains to study the effect of RVE size. (b) Zoom of one of the grains showing the different mesh
refinements.
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Although the above results showed that con-
vergence of the stress distribution is achieved forelement sizes of the order of 0:1 lm, a study of
convergence after microcrack initiation needs to be
carried out. To address this issue, a similar simu-
lation was performed considering a microstructure
with an initial crack. The objective of this study
was also to analyze the crack propagation behav-
ior for different mesh refinements. Fig. 6 shows the
distribution of the four stress component ryy rightafter the tensile pulse is generated in the middle of
the RVE. As expected, the stress concentration
near the crack tip becomes more important for the
fine meshes. Fig. 7(a) shows the velocity at the
back of the RVE (after correction due to the ma-
terial impedances). The pullback signal, right after
the end of the first compressive pulse, for the
coarser meshes (h ¼ 1 and 2 lm), indicates that thecrack propagates at a lower speed than in the case
of the finer meshes. This is confirmed in Fig. 7(b),
where the evolution of the crack length for coarser
meshes is well below the ones for finer meshes.
Here again, convergence is achieved when h ¼ 0:1lm.
For a case with Tmax ¼ 1 GPa and KIC ¼ 2
MPa m1=2, according to Eq. (11) the maximum
allowable element size is h 10 lm. Fig. 8(a) and
(b) shows the evolution of the effective stress
and crack length for two mesh sizes: h ¼ 1 lm and
h ¼ 0:1 lm, respectively. The figure illustrates the
effective stress and crack pattern at various timesafter the tensile pulse is generated in the middle of
the RVE. Even though the stress distribution is
more defined in the case with h ¼ 0:1 lm, the crack
pattern for both meshes is exactly the same. Fig. 9
shows the evolution of the crack density for both
cases (plus a simulation with h ¼ 0:05 lm),
showing clearly that convergence is achieved even
when h ¼ 1 lm in agreement with the requirementset by Eqs. (11) and (16).
In addition to this convergence study, linear
and quadratic interface elements, including two
Fig. 4. Contours of effective stress for six different mesh refinements, at 3.5 ns, right after the tensile pulse develops within the RVE.
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and three quadrature point integration schemes,
have been evaluated. The results have shown no
major difference between each other. Although the
shape functions of the quadratic interface element
are compatible with the shape functions of the six-
noded triangular element, the responses of both
interface elements are similar when only micro-cracking is considered as the main source of in-
elasticity. The difference can be only observed
when geometrical and material nonlinearities are
present in the simulation, such as the case where
there is plasticity near the crack tip zone.
One of the most important features in the an-
alyses is the consideration of grain anisotropy. For
a case without initial defects, glassy phase, poresor any other defect in the microstructure, the only
feature leading to stress concentration at triple
points is grain anisotropy. To reveal the impor-
tance of this effect, simulations with and without
grain anisotropy were carried out. Fig. 10 shows
the evolution of the stress distribution right after
the tensile pulse is generated in the middle of the
RVE for both cases. The results demonstrate that
stress concentration is only present in the case with
grain anisotropy, while the stress distribution is
completely uniform for the isotropic case. Like-
wise, the presence of interface elements does notaffect the uniform stress distribution observed in
the isotropic case.
5. A parametric study
The focus of this section will be the investiga-
tion of various geometrical and physical parame-ters that characterize ceramic microstructures and
their effect on the material response under dynamic
loading. Special attention is placed on requirements
leading to proper finite element simulations in the
context of the proposed model. Microstructures
Fig. 5. Contours of effective stress for different mesh refinements. An initial distribution of flaws has been included to examine the
effect of stress concentration in the finer meshes.
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Fig. 6. Distribution of the stress component ryy for a microstructure with an initial crack. The convergence is clear for the finer meshes
(h ¼ 0:1 and 0.05 lm).
Fig. 7. (a) Velocity histories at the back of the momentum trap for different mesh sizes. (b) Evolution of accumulated crack length for
different mesh sizes. Crack pattern evolution for the finest mesh, at different times, is also shown.
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with an interfacial strength of Tmax 1 GPa areconsidered. Since the element size required for
these interfacial strength is in the range of 1–10
lm, meshes with many grains are employed. The
initial velocity used for this parametric study is
V0 ¼ 86 m/s and the duration of the tensile pulse
was taken as dt ¼ 40 ns.
5.1. Effect of RVE size
Simulations were performed using three differ-
ent RVEs to study the effect of the width of the
computational cell. In all cases the spall region
(RVE high), LRVE, Dt and grain size were kept the
same while the width of the RVE was varied;
namely 50, 100 and 200 lm, respectively. Five setsof interface parameters were examined, viz.,
KIC ¼ 1:7, 4, 6 MPa m1=2 and Tmax ¼ 0:8, 1, 1.2
GPa.
The velocity history at the bottom of the ce-
ramic plate is plotted in Fig. 11. The figure shows a
comparison between the three RVE sizes for two
different ceramics: KIC ¼ 4 MPa m1=2 and Tmax ¼ 1
GPa, and KIC ¼ 6 MPa m1=2 and Tmax ¼ 1 GPa. Inboth cases there is a pronounced pullback signal,
although the slope of the signals is different.
Clearly the RVE width effect is minimum. It can be
observed that the major difference in the pullback
signals occurs due to the differences in KIC. Minor
differences are associated to the RVE widths.
Fig. 8. Evolution of the effective stress and crack pattern for Tmax ¼ 1 GPa in which the required element size is h 10 lm. (a) Coarse
mesh h ¼ 1 lm (b) Fine mesh h ¼ 0:1 lm.
Fig. 9. Evolution of crack density for the case with Tmax ¼ 1
GPa and three different meshes.
H.D. Espinosa, P.D. Zavattieri / Mechanics of Materials 35 (2003) 365–394 375
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Fig. 12 shows the crack pattern evolution forthe three RVEs with KIC ¼ 6 MPa m1=2 and
Tmax ¼ 1 GPa. For the narrowest case, two cracks
initiate at the RVE boundaries at about 161 ns and
then a third crack initiates in the middle of the
RVE at 162 ns. The cracks propagate until they
coalesce forming a major crack. A few grains are
surrounded by the microcracks during the growth
phase. For the second and third RVEs(width ¼ 100 and 200 lm) something similar oc-
curs except that in these cases the first two cracks
do not initiate on the boundaries. At about 162 ns
more cracks nucleate. Coalescence into a major
crack occurs at about 185 ls in all cases.
It can be concluded that the RVE width is di-
rectly related to the periodicity of the problem,
which is strongly linked to the nucleation sites.
Considering that the microcrack initiation siteswill depend on the distribution of grain orienta-
tions, initial defects, stochasticity of grain bound-
ary strength and toughness, and stress wave
amplitude, the size of the computational cell is
basically determined by the distance between nu-
cleation sites. In the three RVEs being analyzed,
the distance between nucleation sites slightly in-
creases as the width of the RVE increases. There-fore, the analyst can identify the RVE size, as a
function of material properties and stress wave
amplitude, by performing this type of simulations.
5.2. Effect of KIC and Tmax
In this section the effect of KIC and Tmax will be
studied separately. An RVE size of 100 lm has
Fig. 10. Contours of effective stress at 3.5 and 4 ns for h ¼ 0:1 lm with and without grain elastic anisotropy.
376 H.D. Espinosa, P.D. Zavattieri / Mechanics of Materials 35 (2003) 365–394
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been utilized for these simulations in order to ob-
tain a reasonable computational time.
5.2.1. Effect of KIC
Initial numerical simulations with KIC ¼ 1:7, 4and 6 MPa m1=2 and Tmax ¼ 1 GPa, were per-
formed. After examination of results and noticing
that the pullback signal was diminished as KIC was
increased, new simulations with higher values of
KIC were performed up to 25 MPa m1=2. Fig. 13(a)
shows the velocity at the back of the specimen for
these simulations with different values of KIC. For
small values of KIC the pullback signal is impor-tant. For KIC ¼ 1:7 the duration of the pullback
signal is close to the duration of the pulse. As KIC
is increased, this duration decreases until KIC
reaches 10 MPa m1=2. For this value of KIC, not
only the pullback signal duration decreases but
also the shape and maximum pullback pulse am-plitude change. For the cases with KIC 6 10, there
is no second compressive pulse. Fig. 13(b) shows
the entire velocity history for KIC P 10 MPa m1=2.
The shape of the second compressive pulse for
KIC ¼ 15 is quite different from the case with
KIC ¼ 20 MPa m1=2, where its duration becomes
larger than the theoretical second compressive
pulse duration due to wave spreading. Fig. 14shows the obtained crack patterns for the various
Fig. 11. Effect of RVE width: three different meshes were used for this study, with two different KIC. The simulations demonstrate that
the RVE size does not play an important role in the velocity history.
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values of KIC. When KIC P 20 m1=2, there is no
evidence of microcracks.
5.2.2. Effect of TmaxIn this subsection we examine the effect of in-
terface strength, Tmax. Fig. 15 shows the velocity
history at the back of the specimen for Tmax ¼ 0:8,1, 1.2, 1.5, 1.6, 1.7, 1.8, 1.9, 2.0 GPa when KIC is
maintained at 4 MPa m1=2. In this figure, only the
end of the first compressive pulse and the pullback
signal is displayed. It is clear from this figure that
the effect of Tmax is not as rich as the effect of KIC
discussed in the previous subsection. Tmax only
governs the depth of the valley, i.e., maximumstress unloading, and has almost no effect on the
shape and duration of the pullback signal. It
should be noted that the macroscopic stress am-
plitude for an initial velocity V0 ¼ 86 m/s is ap-
proximately 1.5 GPa.
When the interface strength, Tmax, reaches this
value no damage is generated in the specimen, and
therefore there is no pullback signal. Fig. 16 showscrack patterns for each one of the cases being ex-
amined. The crack density seems to be smaller for
higher values of Tmax until a threshold stress is
reached. In all cases the width of the spall region is
limited to a couple of grains.
5.2.3. Discussion on the effect of KIC and TmaxAs it was demonstrated earlier, the effect of KIC
seems to be stronger on the shape and duration of
the pullback signal than the effect of Tmax. As KIC
increases, the pullback signal decreases its duration
and changes its shape. As we increase Tmax only the
valley between the first compressive pulse and the
Fig. 12. Evolution of the crack patterns, during spallation, for
three different RVEs with KIC ¼ 6 MPa m1=2 and Tmax ¼ 1 GPa.
The evolution is rather similar in all three cases.
Fig. 13. (a) Effect of KIC on particle velocity at the specimen-momentum trap interface. The higher KIC, the smaller the pullback signal.
(b) Velocity at the specimen-momentum trap interface for KIC ¼ 10–20 MPa m1=2.
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pullback signal changes. In other words, only
partial unloading occurs within the material be-
cause of the generated damage. The pullback signal
disappears when the grain boundary strength Tmax,is equal or higher than the applied macroscopic
stress. Fig. 17 shows the effect of these two pa-
rameters on the crack density evolution. It is
noteworthy how the maximum crack density value,
the crack initiation time, and the evolution rate are
affected by KIC while they barely change as Tmax
varies. Not only the maximum crack density value
decreases as KIC is increased, but also the crackinitiation time is delayed. The crack initiation time
is the same for different values of Tmax.
5.2.4. Synergy between KIC and TmaxUp to this point, the effect of KIC has been
studied for Tmax ¼ 1 GPa and the effect of Tmax
for KIC ¼ 4 MPa m1=2. The idea in this subsec-tion is to present additional simulations com-
bining the variation of both parameters at the
same time in order to study the interaction and
relationship between them. Fig. 18 shows six
different cases or combinations of different values
of KIC and Tmax; namely, KIC ¼ 4, 6 and 8
MPa m1=2 and Tmax ¼ 1, 1.2 and 1.5 GPa. These
simulations clearly show that the thresholdmaximum strength, T th
max, needed for eliminating
damage, is dependent on KIC.
Fig. 14. Effect of KIC on crack pattern.
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5.3. Effect of initial defects
Here the presence of initial microcracks within
the RVE is examined in the context of their effect
on specimen bottom surface velocity. Distribu-
tions of initial defects have been considered with
1% and 5% of interface elements broken. An RVE
size of 100 lm is utilized in the simulations. Theinterface element parameters used in the simula-
tions were Tmax ¼ 2 GPa and KIC ¼ 4 MPa m1=2.
Fig. 19 shows the effect of initial defects within
the RVE. As it was seen in the previous section,
when Tmax ¼ 2 GPa, KIC ¼ 4 MPa m1=2 and the
RVE does not contain initial defects, microcrack-
ing does not occur. Fig. 19 shows that the presence
of initial defects undoubtedly affects the behaviorof the specimen. Damage is not only initiated but
its spreading in the spall region noteworthy. Sim-
ilarly, crack bifurcation is also observed. In the 5%
case, the distance between microcracks, i.e., spall
region width, is reduced. A double pullback signal
is predicted in the 1% case. This feature is quite
interesting and illustrates how significant varia-
tions in crack kinetics can occur.
5.4. Stochastic effects as represented by Weibull
distributions
In this subsection, the Weibull distribution of
Tmax given by Eqs. (53) and (54) in part I has been
considered for T 0max ¼ 1, 2 and 5 GPa and m ¼ 3
and 10. As it is known, m ¼ 3 approximates a
Gaussian distribution, while a value of m ¼ 10 is
typical of some brittle materials. An RVE size of
100 lm and KIC ¼ 4 MPa m1=2 were utilized in the
simulations. Fig. 20(a) shows the two distribu-tions, m ¼ 3 and 10, for T 0
max ¼ 1 together with the
crack pattern after spallation and the velocity
histories at the back of the specimen. Even though
it is not shown in this figure, the velocity history
for the same case without a Weibull distribution,
i.e., uniform strength in the RVE of Tmax ¼ 1 GPa,
is almost identical to the one with m ¼ 10.
A numerical simulation of Weibull distributionswithin the RVE was created, with the help of a
random number generator. The minimum and
maximum values of Tmax in the interfaces were
recorded to compare the various ranges of Tmax
and to check if the values were consistent with the
assumed distributions. For the case of m ¼ 3 the
minimum and maximum values of Tmax are 0.19
and 1.6 GPa, while for the case of m ¼ 10 theminimum and maximum are 0.46 and 1.16 GPa. In
both cases, major cracks develop from side to side
of the RVE and the pullback signal is significant.
No major difference between m ¼ 3 and 10 is ob-
served other than the level of unloading, which is
higher for m ¼ 10 as expected.
Fig. 15. Effect of Tmax on particle velocity at the specimen-
momentum trap interface. In all cases KIC ¼ 4 MPa m1=2.
Fig. 16. Effect of Tmax on the crack pattern after spallation.
380 H.D. Espinosa, P.D. Zavattieri / Mechanics of Materials 35 (2003) 365–394
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Fig. 20(b) shows the two distributions forT 0
max ¼ 2 GPa. It is important to examine the plot
on the upper right hand corner showing the dif-
ferent Weibull distributions for a given T 0max so that
one can appreciate the range of Tmax that is beingconsidered in each analysis. For the case of m ¼ 3,
the minimum and maximum values of Tmax are
0.38 and 3.25 GPa, while for the case of m ¼ 10 the
Fig. 17. Effect of KIC and Tmax on crack density evolution.
Fig. 18. Plots illustrating the synergy between KIC and Tmax.
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minimum and maximum are 0.93 and 2.33 GPa.
This analysis shows a marked difference in the
velocity history and crack pattern for m ¼ 3 and
10. For the case with m ¼ 10 there is a second
compressive pulse, and the formed crack is belowthe expected location for the spall plane. For the
case with m ¼ 3 no second compressive pulse is
observed and the crack propagates from side to
side of the RVE in a much shorter time than the
tensile pulse duration.
Fig. 20(c) shows the distribution used with
T 0max ¼ 5 GPa. For this case only m ¼ 3 has been
plotted because when m ¼ 10 no damage is ob-served. The minimum and maximum values of Tmax
are 0.85 and 9.06 GPa, respectively. The result is
similar to the one for m ¼ 3, T 0max ¼ 2 GPa con-
sistent with the observation that if many interfaces
in the RVE have a Tmax below the macroscopically
applied tensile stress, spallation occurs rather
suddenly and the second compressive pulse dis-
appears.
5.5. Rate dependent microcracking
A rate dependent cohesive surface model is
proposed to examine rate effects during the cre-
ation of the fracture surfaces. In this rate depen-
dent cohesive surface model, the cohesive strength
Tmax is taken to be dependent on the instantaneous
rate of the effective displacement jump, _kk. The
function Tmax ¼ f ð _kkÞ used in this analysis is given
by
Tmax ¼ T 0max 1
þ b2 log
_kk_kkref
" #!ð17Þ
This rate dependent model was proposed by
Espinosa et al. (1998). Another model based on
an exponential law was introduced by Lee and
Prakash (1999) in the study of metals. It should
be mentioned that the exponential law can pre-
sent problems of instabilities due to the sudden
growth of Tmax inherent in the exponential type
function. Hence, care must be exercised in itsimplementation. In fact, high values of Tmax lead
to high initial slopes ðs ¼ Tmax=ðkcrdÞÞ requiring
smaller elements.
For this study, different values of b2 have been
considered. The reference effective displacement
jump rate is chosen as _kkref ¼ 1 � 108/s. The case
with Tmax ¼ 1 GPa and KIC ¼ 4 MPa m1=2 is ex-
amined. Fig. 21(a) shows the velocity history at theback of the specimen for b2 ¼ 2, 8, 10, 15, 20 and
25. The pullback signal is clearly affected by the
value of b2 and it tends to disappear as b2 is in-
creased. Fig. 21(b) shows the crack density evo-
lution for each one of these cases. Contrary to
what one would expect, the maximum value of the
crack density increases with the value of b2. Fig. 22
shows even a more interesting view of this phe-nomenon. The crack pattern spreads and covers
more area of the spall region as b2 is increased. As
the spall region diffuses, the crack pattern is rep-
resented by a uniform distribution of individual
microcracks instead of one major crack as in the
cases with lower values of b2.
Fig. 19. Effect of initial defects, for KIC ¼ 4 MPa m1=2 and
Tmax ¼ 2 GPa, on particle velocity and microcracking. Zero,
one and five percent of broken interface elements were con-
sidered.
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A similar study has been performed for b2 ¼10, 15, 20 and 25, and _kkref ¼ 0:5 � 108 1/s. The
effect of using smaller values of _kkref is similar to
shifting the curves of Tmax=T 0max to the left, which
means that for lower values of _kkref , Tmax is higher
for a fixed _kk. Fig. 23 shows the effect of _kkref for
b2 ¼ 10, 15, 20 and 25. The second compressive
pulse is observed for b2 ¼ 20 and 25, but its
shape is not consistent with experimental results.
In fact, the shape of the second compressive pulseis similar to the ones obtained with very high
values of KIC.
Fig. 20. (a) Weibull distribution f ðTmaxÞ for T 0max ¼ 1 GPa. On the upper right hand corner, both Weibull distributions (m ¼ 3 and 10)
are illustrated. In the same figure the crack pattern and velocity history at the back of the specimen are plotted. (b) Weibull distribution
f ðTmaxÞ for T 0max ¼ 2 GPa. On the upper right hand corner, both Weibull distributions (m ¼ 3 and 10) are illustrated. The crack pattern
and velocity history at the back of the specimen are plotted. (c) Weibull distribution f ðTmaxÞ for T 0max ¼ 5 GPa. On the upper right hand
corner, both Weibull distributions (m ¼ 3 and 10) are illustrated. In the same figure the crack pattern and velocity history at the back of
the specimen are plotted.
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Fig. 24(a) shows this effect on the evolution ofthe crack density. The crack initiation time is de-
layed for smaller values of _kk while the slope re-
mains almost identical, except that the maximum
crack density behaves differently for both _kkref .
Contrary to what happens with _kkref ¼ 1:0 � 108/s,
in the case with _kkref ¼ 0:5 � 108/s the maximum
crack density decreases as b2 is increased. Fig.
24(b) shows the crack pattern for each b2 and_kk ¼ 0:5 � 108/s. The behavior observed in theprevious case, now it is more pronounced leading
to a diluted crack pattern when b2 ¼ 25. It should
be noted that such crack pattern is not consistent
with experimental observations (Espinosa et al.,
1992).
6. Simulations with high values of Tmax (strong
ceramics and composites)
High purity ceramics are synthesized such that
their grain boundary strength can reach values ofabout E=40 or even E=20. In this section a para-
metric study of the effect of cohesive law parame-
ters is given when Tmax ¼ 10 GPa. The initial
velocity is chosen to be V0 ¼ 92 m/s and the pulse
duration dt ¼ 25 ns; these values correspond to
one of the experiments performed by Raiser et al.
(1994). The purpose of this study is to demonstrate
that the effect of various model parameters are
Fig. 21. (a) Espinosa�s rate dependent model prediction of velocity histories for b2 ¼ 2, 8, 10, 15, 20 and 25, and _kkref ¼ 1 � 108 1/s. (b)
Evolution of crack density for different values of b2 and _kkref ¼ 1 � 108 1/s.
Fig. 22. Effect of b2 on crack pattern.
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similar to what was presented when Tmax 1 GPa.
Unique and interesting features are observed in the
case of strong ceramics.
As discussed in the convergence analysis, when
high values of Tmax are examined, e.g., Tmax ¼ 10GPa and KIC ¼ 2 MPa m1=2, the element size re-
quired for simulations is in the range h ¼ 0:1–0.2
lm. This means that the analyst will have to
carefully select the appropriate RVE to limit the
computational time. The principal factors for this
choice are
1. Periodicity: The periodicity of the problem, andtherefore the width W of the RVE is linked to
the distance between crack nucleation sites.
This periodicity does not depend only on the
geometry (grain shape and size, distribution of
initial flaw, pores or glassy phase) but also
depends on the loading conditions (impact
velocity V0, and pulse duration dt).2. Extent of microcracking: It was experimentally
observed that microcracks propagate and co-
alesce in the so-called spall region (Espinosa et al.,
1992); this spall region depends on the grain size
and morphology. Typically, microcracks propa-
gate in a region consisting of two or three grains
above and below the spall plane. However, the
height H of the RVE has to be chosen such
that there are several rows of grains betweenthe spall region and the top and bottom bound-
aries in order to avoid boundary effects aris-
ing from condition of uniform displacement
and velocity imposed by the viscous boundary
conditions representing the homogenized ce-
ramic.
In the following subsections a parametric study
is presented with an RVE size of 20 � 20 lm2 and
a grain size of 2 lm (10 � 10 grains). The interface
strength considered in all these cases is chosen to
be Tmax E=40 ¼ 10 GPa. In some cases the width
of the RVE is enlarged to study the effect of pe-
riodicity on crack nucleation, propagation and
coalescence.
6.1. Effect of crack initiation distance on propaga-
tion and branching
In this study, the crack propagation pattern is
enriched by a stochastic distribution of grain
boundary strength and toughness. The Weibull
parameters used in the simulations were: T 0max ¼ 10
GPa, K0IC ¼ 2 MPam1=2 and m ¼ 10. An initial
crack of a few microns is considered on the side of
the RVE. Three RVEs are considered, the height is
20 lm in all the cases while the width is 20, 40 and60 lm, respectively. The idea of considering dif-
ferent RVE width with only one initial crack is to
study the effect of nucleation sites distance on
material response.
Fig. 25 shows the crack pattern and stress (ryy)
evolution for the case with an RVE of 60 � 20
Fig. 23. Espinosa�s rate dependent model prediction of velocity histories for b2 ¼ 10, 15, 20 and 25, and _kkref ¼ 0:5 � 1081=s.
H.D. Espinosa, P.D. Zavattieri / Mechanics of Materials 35 (2003) 365–394 385
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Fig. 24. (a) Evolution of the crack density using the rate dependent model and various values of b2 and _kkref ¼ 0:5 � 108 1/s. (b) Effect
of b2 on the crack pattern.
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lm2. The crack starts propagating at 3 ns (when
the tensile pulse reaches the spall plane) and
propagates until coalescence. Crack branching is
observed at 5 ns. Fig. 25 clearly shows the stress
concentration at the crack tips for each branch.
The effect of distance between nucleation sites, for
the different RVEs, is illustrated in Figs. 26 and 27.
The 20 � 20 lm2 RVE corresponds to a case
where there is a nucleating crack every 20 lm, the
40 � 20 lm2 RVE corresponds to the case where
Fig. 25. Evolution of ryy on a 60 � 20 lm2 RVE containing an initial crack. The tensile pulse develops at 3 ns and it propagates
through the ceramic until crack coalescence.
Fig. 26. Effect of distance between crack nucleation sites on velocity history and crack length evolution.
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there is a nucleating crack every 40 lm, and the
60 � 20 lm2 RVE to the case where there is a
nucleating crack every 60 lm. By examining the
crack length history, Fig. 26 (right), one can notice
that although the initial slope of the accumulated
crack length is almost the same for all three cases,
the pullback signal is more pronounced in the casewith the highest density of nucleation sites, i.e.,
nucleation sites every 20 lm. These findings illus-
trate the fact that the pullback signal represents a
combination of two factors, the crack speed and
the time the crack takes to coalesce with its
neighbors.
Fig. 27 shows the crack pattern evolution for
each one of the three cases. For the 20 � 20 lm2
RVE, crack branching is inhibited, because co-
alescence occurs before the onset of branching.
For the 40 � 20 and 60 � 20 lm2 RVEs, the
crack branches and the degree of branching
is more pronounced for the largest RVE, i.e.,
when the distance between nucleating sitesincreases.
Fig. 28 illustrates rate effects for the 40 � 20
lm2 RVE. Even though the accumulated crack
length history seems to be significantly dependent
on b2 (hereafter b), the velocity history is not
strongly affected when b 0:1. In fact, Fig. 29
shows the evolution of the crack pattern for the
various cases. An interesting observation is thatrate effects delay and/or inhibit crack branching.
This feature explains the observed differences in
accumulated crack length evolution. The speed at
which the crack propagates and coalesce, with
neighbor cracks, does not seem to change with rate
effects, but the capability of the ceramic to branch
does. The variation on the accumulated crack
length evolution is due to this factor. The crackaccumulated length is reduced as b increases. A
similar effect is observed for different values of KIC.
Fig. 30 shows how branching tends to disappear
when KIC increases. The similarity between rate
effects and toughness, on the pull back signal, were
previously highlighted. As one would expect, crack
branching in the form of a ‘‘funnel’’ is not only
dependent on rate effects but also on the value ofKIC, which is directly related to the dissipated en-
ergy at the interfaces. This means that in low
toughness ceramics, branching will be more likely
than in ceramics with tough interfaces where the
energy needed to create new surfaces is higher. It is
important to keep in mind that stochasticity of the
microstructure would make these patterns vary
according to the different grain geometry andorientation, interface strength distribution, pres-
ence of initial defects, etc. If a considerable num-
ber of simulations with different grain orientations
and interface strength distribution is carried out, a
set of parameters for which crack branching would
occur can be obtained. It should be noted that this
kind of behavior is also observed for cases with
single cracks. Ballarini (2000), observed that for asingle crack a ‘‘funnel’’ like zone can be defined
considering the stochasticity of the microstructure.
Fig. 27. Crack pattern evolution for three different RVEs.
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Fig. 28. Rate effects on velocity history for the 40 � 20 lm2 RVE.
Fig. 29. Rate effects on crack pattern evolution for the 40 � 20 lm2 RVE.
H.D. Espinosa, P.D. Zavattieri / Mechanics of Materials 35 (2003) 365–394 389
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6.2. Modeling residual thermal stresses and induced
microcracking
Throughout the analyses discussed in previoussections, the ceramic microstructure has been ide-
alized as an ensemble of randomly oriented, elas-
tically and thermally anisotropic grains with brittle
intergranular interfaces. Nonetheless, thermal
stresses and microcracking resulting from the
material fabrication process were not considered.
Fig. 30. Effect of KIC on velocity history, crack length evolution and crack pattern.
390 H.D. Espinosa, P.D. Zavattieri / Mechanics of Materials 35 (2003) 365–394
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It is well known that in the sintering of ceramics,
the material is brought from its fabrication tem-perature down to room temperature. In some ce-
ramics, the stresses in the sample are partially
relaxed, during cooling, due to creep along grain
boundaries.
Since quasi-static simulations of the residual
thermal stresses during cooling in the process of
fabrication have been performed in the past, (Ev-
ans, 1978; Fu and Evans, 1985; Tvergaard andHutchinson, 1988; Ortiz and Suresh, 1993; Sridhar
et al., 1994), in this section we just present the ef-
fect of residual thermal stresses on the dynamic
behavior of the ceramic.Fig. 31 shows the effect of the residual stresses
corresponding to a drop of 1500� K during the
material fabrication process. The Weibull para-
meters are T 0max ¼ 10 GPa, K0
IC ¼ 2 MPam1=2 and
m ¼ 1. Since the overall effect of the thermal re-
sidual stresses has been observed to be similar for
different Weibull parameters, we have chosen these
parameters for our discussion purposes. These sim-ulations and others considering different cohesive
properties, did not result in a marked tendency of
Fig. 31. Effect of thermal residual stress on velocity history, crack length evolution and crack pattern. Histograms of ryy and reff are
also included in the figure to illustrate shift due to residual stresses.
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the material behavior. In some cases the ceramic
seems to be stronger when the residual stresses are
superimposed. Histograms of ryy and reff for each
case have been obtained to study this phenomena.
It was observed that bigger RVEs need to be
considered to obtain statistically significant results.In all cases the thermal stresses introduce a pertur-
bation on the histogram of stresses when compared
to the cases without thermal stresses, see Fig. 31.
Such perturbation is not enough to significantly
change the overall material dynamic behavior. In
fact, the perturbations in stress are about 20–100
MPa, which appear to be small when compared to
the applied macroscopic stress of about 1 GPa tosignificantly affect the onset of microcracking and
its evolution. It is expected that residual thermal
stresses may affect the threshold stress required for
crack initiation as well as the location of initial
defects in the material microstructure but do not
seem to result in a significant departure from the
features observed in the absence of residual stres-
ses. These findings validate all the analyses andconclusions obtained in the absence of residual
stresses.
7. Concluding remarks
In this paper, the micromechanical model in-
troduced in part I was used to simulate wavepropagation experiments. The numerical results
are shown in terms of microcrack patterns, evo-
lution of crack density, and velocity histories
simulated at the back of the ceramic plate. Two
parametric studies were performed, one for
Tmax 1 GPa (weak ceramics) and another for
Tmax 10 GPa (strong ceramics). To reduce the
calculation time without changing the physics ofthe problem, a simplified model has been proposed
and implemented. The effect of RVE size was
studied along with different interface properties.
Conditions under which solution convergence is
obtained were derived and illustrated in Section
5.5.
Section 5.2 illustrates the effect of KIC and
Tmax, in the absence of stochasticity and rate ef-fects, on the macroscopic material response. The
most important conclusion from this section is
that KIC affects significantly the crack density
evolution, crack pattern and pullback signal,
while changes in grain boundary strength, Tmax do
not significantly affect damage evolution as long
as Tmax is below the applied macroscopic tensile
stress. It is also noteworthy that the pullbacksignal decreases for high values of KIC and that
the second compressive pulse is much wider than
the second compressive pulse predicted by elastic
wave theory. It should be noticed that even when
no cracks are observed on plotted crack patterns,
damage is present in the form of energy dissipa-
tion in the interface elements (when T > Tmax and
k < 1). The way in which the energy is dissipatedon the interface elements changes the shape of the
second compressive pulse. Furthermore, the val-
ues of KIC for which the pullback signal totally
disappears are unrealistic for ceramic materials,
i.e., KIC ¼ 20–25 MPa m1=2.
Section 5.3 outlines the effect of initial defects.
Different percentages of initial defects were con-
sidered. It was observed that, in some cases, thecracks do not propagate along the expected spall
plane. When a spall plane is formed, distinct fea-
tures such as formation of double major cracks
and branching are observed. Section 5.4 shows the
effect of considering a Weibull distribution on Tmax
while keeping KIC constant. A study of various
T 0max, m (Weibull parameter) and different fixed KIC
were performed. A range of responses was ob-tained for different sets of parameters. It was also
observed that for a given set of parameters, but
different seeds, the response changes significantly.
The extreme case occurs for a distribution of Tmax
in which some interfaces exhibit Tmax ¼ 0.
Finally, in Section 5.5 a parametric study of rate
dependent models was carried out. For the con-
sidered law, the bigger the parameter b2 is, thehigher the Tmax growth rate. Also, the smaller the_kkref , the higher the Tmax growth rate. The most im-
portant finding was that for higher rate effects
(which means for higher values of b2 or/and smaller
values of _kkref ) the crack pattern presents isolated
microcracks distributed on a wide region, while for
smaller rate effects the microcracks concentrate
very close to the crack plane approaching, asymp-totically, the case without rate effects in which only
one major crack forms.
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In addition the following features have been
identified:
1. The distribution of Tmax in the RVE controls
maximum unloading and the onset of damage
while KIC strongly affects damage kinetics. Thepullback signal disappears for very high values
of KIC but the shape of the second compressive
pulse is not consistent with experimental re-
sults. All possible combinations of Tmax and
KIC have been considered and no set of para-
meters has been found to adequately reproduce
experimental results. Therefore, other micro-
structural features, such as nonuniform grainsize and shape distributions, need to be in-
cluded to capture the velocity histories and
crack patterns observed in experiments (Zavat-
tieri and Espinosa, 2001).
2. The effect of introducing a Weibull statistics is
only important for some values of Tmax. If the
value of T 0max is not close to a representative va-
lue for the material, statistical fluctuations arenot important. For low values of T 0
max the ce-
ramic presents the same damage almost inde-
pendently of the distributions, while for high
values of T 0max the ceramic did not exhibit any
damage.
3. Initial defects only affect the cases for which the
interface strength, Tmax is in excess of the ap-
plied stress amplitude. The velocity historiesand crack patterns change depending on the in-
terface parameters. In some cases microcracks
do not initiate at the spall plane. The percentage
of initial flaws becomes more relevant as the va-
lue of Tmax increases.
4. Rate effects eliminate the pullback signal (for
relative small values of KIC). However, the be-
havior of the second compressive pulse is simi-lar to the ones found for high values of KIC.
Crack patterns are significantly affected leading
to cases where the spall region is defined by a
diffused set of isolated microcracks.
5. It was shown that the RVE size is determined
by the properties of the ceramic and the ampli-
tude of the stress wave. The lower the amplitude
of the applied stress pulse, the larger the RVEneeds to be such that all possible values of inter-
face strength and toughness are manifested
within the RVE. The minimum RVE size can
be consistently determined using the methodol-
ogy presented in this work.
Acknowledgements
The authors acknowledge ARO and DoD
HPCMP for providing supercomputer time on the
128 processors Origin 2000 at the Naval Research
Laboratory––DC (NRL-DC). This research was
supported by the National Science Foundation
through Awards no. CMS 9523113 and CMS-9624364 (NSF-CAREER), the Office of Naval
Research YIP through Award no. N00014-97-1-
0550, the Army Research Office through ARO-
MURI Award no. DAAH04-96-1-0331 and the
Air Force Office of Scientific Research through
Award no. F49620-98-1-0039.
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